The Oscillating Universe: an Alternative to Inflation
Ruth Durrer (D\'epartement de Physique Theorique, Universit\'e de, Gen\`eve), Joachim Laukenmann (Institut f\"ur Theoretische Physik,, Universit\"at Z\"urich)

TL;DR
This paper explores the oscillating universe model as a viable alternative to inflation, addressing key cosmological problems and analyzing density perturbations to understand the universe's large-scale structure.
Contribution
It demonstrates that the oscillating universe can solve flatness, entropy, and horizon issues, and provides a framework to test universe geometry through power spectrum measurements.
Findings
Oscillating universe addresses flatness, entropy, and horizon problems.
Density perturbation evolution constrains previous cycle characteristics.
Large-scale power spectrum measurements can determine universe geometry.
Abstract
The aim of this paper is to show, that the 'oscillating universe' is a viable alternative to inflation. We remind that this model provides a natural solution to the flatness or entropy and to the horizon problem of standard cosmology. We study the evolution of density perturbations and determine the power spectrum in a closed universe. The results lead to constraints of how a previous cycle might have looked like. We argue that most of the radiation entropy of the present universe may have originated from gravitational entropy produced in a previous cycle. We show that measurements of the power spectrum on very large scales could in principle decide whether our universe is closed, flat or open.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
